We provide an updated scan of the allowed parameter space of the two-loop Zee-Babu model for neutrino mass. Taking into account most recent experimental data on $\mu\to e\gamma$ as well as the mixing angle $\theta_{13}$ we obtain lower bounds on the masses of the singly and doubly charged scalars of between 1 to 2 TeV, with some dependence on perturbativity and fine-tuning requirements. This makes the scalars difficult to observe at LHC with 14 TeV even with optimistic assumptions on the luminosity, and would require a multi-TeV linear collider to see the scalar resonances. We point out, however, that a sub-TeV linear collider in the like-sign mode may be able to observe lepton flavour violating processes such as $e^- e^- \to \mu^- \mu^-$ d...
AbstractIn this talk we discuss how the Zee-Babu model can be tested combining information from neut...
An extension of the Zee model involving a light right handed neutrino, nu_R is considered. We update...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
We provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for neutrin...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
AbstractIn this talk we discuss how the Zee-Babu model can be tested combining information from neut...
In this talk we discuss how the Zee-Babu model can be tested combining information from neutrino dat...
Contrary to the see-saw models, extended Higgs sectors leading to radiatively-induced neutrino masse...
AbstractWe update previous analyses of the Zee–Babu model in the light of new data, e.g., the mixing...
Motivated by searches for so-called leptonic scalars at the LHC and the recent measurement of the $W...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
AbstractIn this talk we discuss how the Zee-Babu model can be tested combining information from neut...
An extension of the Zee model involving a light right handed neutrino, nu_R is considered. We update...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
We provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for neutrin...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
AbstractIn this talk we discuss how the Zee-Babu model can be tested combining information from neut...
In this talk we discuss how the Zee-Babu model can be tested combining information from neutrino dat...
Contrary to the see-saw models, extended Higgs sectors leading to radiatively-induced neutrino masse...
AbstractWe update previous analyses of the Zee–Babu model in the light of new data, e.g., the mixing...
Motivated by searches for so-called leptonic scalars at the LHC and the recent measurement of the $W...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
AbstractIn this talk we discuss how the Zee-Babu model can be tested combining information from neut...
An extension of the Zee model involving a light right handed neutrino, nu_R is considered. We update...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...